1432-0033: new campaign target copy of [vsnet-alert 5037, T. Vanmunster]: Dear colleagues, I'm observing the dwarf nova 1432-0033 in response to the recent = outburst reported by R. Stubbings (VSNET-ALERT 5030), using the 0.35-m = f/6.3 telescope with unfiltered ST-7 CCD of CBA Belgium Observatory. = Also running my "real-time" light curve generator, allowing on-the-fly = CCD data reduction and light curve visualisation. The light curve clearly shows a superhump-like profile with an amplitude = of about 0.6 mag. It's very difficult to determine the period of the = signal (given the noise due to the low altitude of the object). A guess, = looking at the light curve on screen, yields a value of approx. 0.07 d. In Astrophys. J. Sup. 78, 409, 1992, Berg et al. mentioned this object = as an emission-line CV, with a "resemblance to HT Cas and U Gem". The = object is located at 14h32m25.88s, -00d33'00".9 (J2000), with a reported = quiescent magnitude of 18.5 I'll continue monitoring this object as long as possibe (but already = getting very low now). Assistance from other observatories would be = appreciated. Best regards, Tonny === The object is naturally brought to the VSNET campaign program! Please continue to keep a watch! Judging from the large amplitude of superhumps, the system might be a (grazing) eclisper. Regards, Taichi Kato